在亚暴期间能量是如何进入磁层的:经过60年的实地研究后的观点

G. Haerendel
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引用次数: 0

摘要

本文首先概述了我进入空间物理学的道路以及随后四十年来在电离层和磁层的积极研究。下面的透视部分分四个步骤阐述了主要问题,从亚暴开始前的气流制动和转向,通过由气流爆发携带的磁场的附着,到进入的动量和能量的转换及其向地球传播,最后,产生极向弧,极光电喷流和亚暴电流楔。这主要是通过对作者1992年至2021年研究成果和概念的批判性评估来完成的。其结果是一个新的情景的起源的分裂弧,极光电喷流和亚风暴电流楔。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
How Energy Enters the Magnetosphere During a Substorm: A Perspective After 60 Years of Working in the Field
This paper begins with a summary of my path into space physics and the following four decades of active research in ionosphere and magnetosphere. The following perspective part addresses the main subject in four steps, from flow braking and diversions prior to substorm onset, via the attachment of the magnetic field carried by the flow bursts, to the transformation of the incoming momentum and energy and their earthward propagation, and finally, the generation of the poleward arcs, auroral electrojet, and substorm current wedge. This is done mostly by a critical assessment of results and concepts from the author's research from 1992 to 2021. The outcome is a new scenario of the origin of the breakup arcs, auroral electrojet, and substorm current wedge.
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